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Studying the evolution of the contamination of the Sunyaev-Zel'dovich effect due to high-redshift (sub-)mm galaxies

Montana, Alfredo, Aretxaga, I., Austermann, J., Bock, J., Chapin, E., Gaztanaga, E., Hughes, D., Lowenthal, J., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Perera, T., Scott, K., Wilson, G. and Yun, M. 2007. Studying the evolution of the contamination of the Sunyaev-Zel'dovich effect due to high-redshift (sub-)mm galaxies. Presented at: AAS/AAPT Joint Meeting 2007, Seattle, WA, USA, 5-10 Jan 2007. Bulletin of the American Astronomical Society. Bulletin of the American Astronomical Society (38) American Astronomical Society, p. 267.

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Abstract

We present simulations of the submillimetre/millimetre (sub-mm) sky to study the environment of luminous starburst galaxies, radio galaxies and AGN towards biased-regions (large-scale over-densities) in the high-redshift universe. Guided by recent results from AzTEC extragalactic surveys at 1.1mm, we describe the impact of this population of galaxies, that dominate the sub-mm extragalactic background, on the detectability of the Sunyaev-Zel'dovich effect (SZE) as a function of redshift. These results will be presented in the context of the next generation of wide-area surveys to identify high-redshift clusters via the SZE.

Item Type: Conference or Workshop Item (Poster)
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Publisher: American Astronomical Society
ISSN: 0002-7537
Related URLs:
Last Modified: 27 Oct 2022 10:09
URI: https://orca.cardiff.ac.uk/id/eprint/69113

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